SDO HMI 2011-05-05 20:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.14 | 368.89 | 48.05 | 195.07 | 16.50 | 48.14 | -1.14 | 3.00 | 0.3500 | -334.8 | 0.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.43 | 0.00 | 0.78 | 20.84 | 53.78 | 4.50 | 350.00 | 0.4238 | 748.0 | 570.6 | |
| 0.00 | 1.52 | 0.00 | 0.81 | 18.11 | 53.29 | 4.01 | 349.87 | 0.3793 | 770.0 | 627.6 | |
| 0.00 | 0.98 | 0.00 | 0.51 | 15.20 | 51.00 | 1.72 | 354.89 | 0.3270 | -892.0 | -743.8 | |
| 1.97 | 197.10 | 1.04 | 104.00 | 16.09 | 50.35 | 1.07 | 356.98 | 0.3410 | -1081.0 | -404.5 | |
| 10.10 | -4.00 | 5.33 | -4.00 | 16.54 | 50.22 | 0.94 | 357.39 | 0.3483 | -977.8 | 999999 | |
| 25.46 | -4.00 | 13.42 | -4.00 | 16.16 | 49.91 | 0.63 | 358.23 | 0.3417 | -1178.9 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 17.22 | 49.85 | 0.57 | 358.48 | 0.3592 | 209.0 | 178.9 | |
| 25.20 | 32.25 | 13.23 | 16.94 | 15.64 | 49.44 | 0.16 | 359.55 | 0.3331 | -1105.4 | -744.1 | |
| 9.02 | -4.00 | 4.76 | -4.00 | 16.22 | 49.18 | -0.10 | 0.27 | 0.3426 | -1009.0 | 999999 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 16.29 | 48.68 | -0.60 | 1.68 | 0.3438 | -662.0 | -517.4 | |
| 3.84 | 6.52 | 2.02 | 3.43 | 15.74 | 48.49 | -0.79 | 2.27 | 0.3349 | -722.9 | -445.0 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 22.10 | 48.14 | -1.14 | 2.43 | 0.4379 | 783.0 | 611.4 | |
| 0.00 | 1.43 | 0.00 | 0.75 | 16.03 | 47.89 | -1.39 | 3.93 | 0.3403 | -680.0 | -539.9 | |
| 0.00 | 3.93 | 0.00 | 2.12 | 19.51 | 47.77 | -1.51 | 3.60 | 0.3969 | -625.0 | -535.8 | |
| 0.00 | 2.14 | 0.00 | 1.13 | 15.87 | 47.77 | -1.51 | 4.32 | 0.3378 | -590.0 | -487.8 | |
| 0.00 | 1.61 | 0.00 | 0.85 | 15.90 | 47.24 | -2.04 | 5.83 | 0.3391 | -714.0 | -597.8 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 16.71 | 47.23 | -2.05 | 5.61 | 0.3523 | -783.0 | -547.2 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 16.16 | 46.76 | -2.52 | 7.08 | 0.3442 | -733.0 | -572.0 | |
| 1.43 | 8.67 | 0.76 | 4.62 | 17.68 | 45.91 | -3.37 | 8.72 | 0.3708 | 935.4 | 746.2 | |
| 0.00 | 6.43 | 0.00 | 3.42 | 17.29 | 45.64 | -3.64 | 9.61 | 0.3652 | 1069.0 | 905.9 | |
| 4.11 | 58.70 | 2.18 | 31.15 | 17.13 | 45.16 | -4.12 | 10.91 | 0.3640 | 1116.1 | 783.4 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 16.10 | 44.81 | -4.47 | 12.46 | 0.3487 | 884.0 | 655.9 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 17.27 | 44.72 | -4.56 | 11.98 | 0.3676 | 863.0 | 637.4 | |
| 0.00 | 2.32 | 0.00 | 1.23 | 17.01 | 44.60 | -4.68 | 12.45 | 0.3639 | 871.0 | 774.5 | |
| 5.45 | -21.00 | 2.89 | -21.00 | 16.68 | 44.57 | -4.71 | 12.71 | 0.3588 | 1135.1 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.14 | 17.37 | 44.33 | -4.95 | 12.89 | 0.3705 | 869.0 | 718.1 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 18.34 | 44.24 | -5.04 | 12.52 | 0.3863 | 634.0 | 487.2 | |
| 0.00 | 4.20 | 0.00 | 2.24 | 17.59 | 44.17 | -5.11 | 13.16 | 0.3747 | 637.0 | 613.0 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 16.91 | 44.12 | -5.16 | 13.72 | 0.3642 | 899.0 | 776.1 | |
| 2.77 | 10.99 | 1.47 | 5.82 | 16.30 | 44.04 | -5.24 | 14.36 | 0.3548 | 1100.0 | 855.8 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 17.37 | 43.92 | -5.36 | 13.93 | 0.3721 | 650.0 | 543.8 | |
| 0.00 | 2.68 | 0.00 | 1.42 | 16.75 | 43.75 | -5.53 | 14.80 | 0.3632 | 776.0 | 681.6 | |
| 0.00 | 2.41 | 0.00 | 1.28 | 16.46 | 43.69 | -5.59 | 15.15 | 0.3588 | 784.0 | 659.5 | |
| 1.79 | -30.00 | 0.95 | -30.00 | 16.17 | 43.67 | -5.61 | 15.44 | 0.3544 | 812.8 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.14 | 16.82 | 43.49 | -5.79 | 15.40 | 0.3653 | 819.0 | 621.0 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.70 | 43.46 | -5.82 | 14.82 | 0.3791 | 877.0 | 709.5 | |
| 0.00 | 2.77 | 0.00 | 1.49 | 18.46 | 41.83 | -7.45 | 18.06 | 0.3983 | 962.0 | 688.3 | |
| 0.00 | 1.43 | 0.00 | 0.78 | 19.18 | 41.67 | -7.61 | 17.84 | 0.4100 | 679.0 | 516.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |